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Ground-Based and Space Observations of Interacting Binaries

Published online by Cambridge University Press:  23 April 2012

Panagiotis G. Niarchos*
Affiliation:
Department of Astrophysics, Astronomy and Mechanics, National and Kapodistrian University of Athens, Athens, Greece email: [email protected]
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Abstract

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Multi-wavelength observational data, obtained from ground-based and space observations are used to compute the physical parameters of the observed Interacting Binaries (IBs) and study the interactions and physical processes in these systems. In addition, the database of IBs from ground-based surveys and space missions will provide light curves for many thousands of new binary systems for which extensive follow up ground-based observations can be carried out. In certain cases, light curves of superior quality will allow studies of fine effects of stellar activity and very accurate determination of stellar parameters. Moreover, many new discoveries of interesting systems are expected from ground-based all-sky surveys and space missions, including low mass binaries and star-planet binary systems. The most important current and future programs of observations of IBs from ground and space are presented.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

Adame, L. et al. , 2011, ApJ, 726, L3CrossRefGoogle Scholar
Andersen, J. 1991, A&AR, vol. 3, No 2, 91Google Scholar
An, J. H. et al. , 2004, MNRAS, 351, 1071CrossRefGoogle Scholar
Bayne, G. et al. , 2002, MNRAS, 331, 609CrossRefGoogle Scholar
Belczyński, K. et al. , 2000, A&AS, 146, 407Google Scholar
Coughlin, J. L., Harrison, T. E., & Gelino, D. M. 2010, ApJ, 723, 1351CrossRefGoogle Scholar
Devor, J. 2005, ApJ, 628, 411CrossRefGoogle Scholar
Fliri, J. et al. , 2006, MmSAI, 77, 332Google Scholar
Gansicke, B. T. et al. , 2006, Ap&SS, 306, 177Google Scholar
Gettel, S. J., Geske, M. T. & McKay, T. A. 2006, AJ, 131, 621CrossRefGoogle Scholar
Hadrava, P. 2006, Ap&SS, 304, 337Google Scholar
Kreiner, J. M. et al. , 2006, Ap&SS, 304, 71Google Scholar
Malkov, O. Yu. et al. , 2006, A&A, 446, 785Google Scholar
Mazeh, T. & Zucker, S. 1994, Ap&SS, 212, 349Google Scholar
Miller-Jones, J. C. A. 2008, JPhCS 131, 012057Google Scholar
Niarchos, P., Munari, U., & Zwitter, T. 2007, in: Hartkopf, W. I., Guinan, E. F., & Harmanec, P. (eds.), Binary Stars as Critical Tools & Tests in Contemporary Astrophysics (Proceedings of IAU Symposium 240, 22-25 August 2006, Prague), p. 244Google Scholar
Paczynski, B. et al. , 2006, MNRAS, 368, 1311CrossRefGoogle Scholar
Pollacco, D. L. et al. , 2006, PASP, 118, 1407CrossRefGoogle Scholar
Pribulla, T. et al. , 2010, AN, 331, 397Google Scholar
Prša, A. & Zwitter, T. 2005, ApJ, 628, 426CrossRefGoogle Scholar
Ritter, H. & Kolb, U. 2003, A&A, 404, 301Google Scholar
Silvestri, N. M. et al. , 2007, AJ, 134, 741CrossRefGoogle Scholar
Stanek, K. et al. , 1998, AJ, 115, 1894CrossRefGoogle Scholar
Vilardel, F., Ribas, I., & Jordi, C. 2006, A&A, 459, 321Google Scholar
Zavala, R. T. et al. , 2010, ApJ, 715, L44CrossRefGoogle Scholar